Fundamental differences between SPH and grid methods

Monthly Notices of the Royal Astronomical Society

Volumn 380, Issue 3, 2007, Pages 963-978

  Agertz, Oscar ^a   Moore, Ben ^a   Stadel, Joachim ^a   Potter, Doug ^a   Miniati, Francesco ^b   Read, Justin ^a   Mayer, Lucio ^b   Gawryszczak, Artur ^c   Kravtsov, Andrey ^d   Nordlund, Åke ^e   Pearce, Frazer ^f   Quilis, Vicent ^g   Rudd, Douglas ^d   Springel, Volker ^h   Stone, James ⁱ   Tasker, Elizabeth ^j   Teyssier, Romain ^k   Wadsley, James ^l   Walder, Rolf ^b  

^a UNIVERSITY OF ZURICH   (Switzerland)

^b ETH ZURICH   (Switzerland)

^c NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^d UNIVERSITY OF CHICAGO   (United States)

^e UNIVERSITY OF COPENHAGEN   (Denmark)

^f UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^g UNIVERSITY OF VALENCIA   (Spain)

^h MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

ⁱ PRINCETON UNIVERSITY   (United States)

^j Columbia University ^*  (United States)

^k CENTRE D ETUDES DE SACLAY   (France)

^l MCMASTER UNIVERSITY   (Canada)

more..

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: general; Hydrodynamics; Instabilities; ISM: clouds; Methods: numerical; Turbulence

Indexed keywords

ASTROPHYSICS; GALAXIES; NUMERICAL METHODS;

COMPARISON STUDY; GALAXIES GENERAL; GALAXY EVOLUTION; GALAXY FORMATIONS; GRID METHODS; ISM : CLOUDS; METHOD: NUMERICAL; PERFORMANCE; SMOOTHED PARTICLE HYDRODYNAMICS; SMOOTHED PARTICLE HYDRODYNAMICS METHODS;

HYDRODYNAMICS;

EID: 34548640111     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12183.x     Document Type: Article

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